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arXiv · gr-qc/9902008

The Inner Structure of Black Holes

Shahar Hod·Tsvi Piran
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Abstract

We study the gravitational collapse of a self-gravitating charged scalar-field. Starting with a regular spacetime, we follow the evolution through the formation of an apparent horizon, a Cauchy horizon and a final central singularity. We find a null, weak, mass-inflation singularity along the Cauchy horizon, which is a precursor of a strong, spacelike singularity along the $r=0$ hypersurface. The inner black hole region is bounded (in the future) by singularities. This resembles the classical inner structure of a Schwarzschild black hole and it is remarkably different from the inner structure of a charged static Reissner-Nordström or a stationary rotating Kerr black holes.

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Shahar Hod, Tsvi Piran. 1999-02-02. The Inner Structure of Black Holes. https://doi.org/10.1023/a%3A1026654519980

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